Distance determination for RAVE stars using stellar models II: Most likely values assuming a standard stellar evolution scenario
The RAdial Velocity Experiment (RAVE) is a spectroscopic survey of the Milky Way. We use the subsample of spectra with spectroscopically determined values of stellar parameters to determine the distances to these stars. The list currently contains 235,064 high quality spectra which show no peculiari...
Prif Awduron: | Zwitter, T, vc, G, Breddels, M, Smith, M, Helmi, A, Munari, U, Bienaymé, O, Binney, J, Bland-Hawthorn, J, Boeche, C, Brown, A, Campbell, R, Freeman, K, Fulbright, J, Gibson, B, Gilmore, G, Grebel, E, Navarro, J, Parker, Q, Seabroke, G, Siebert, A, Siviero, A, Steinmetz, M, Watson, F, Williams, M |
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Fformat: | Journal article |
Iaith: | English |
Cyhoeddwyd: |
2010
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Eitemau Tebyg
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Distance determination for RAVE stars using stellar models: II. Most likely values assuming a standard stellar evolution scenario
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models
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Distance determination for RAVE stars using stellar models
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